Evolution of rotationally and tidally distorted low-mass, close binary systems - Implications for the minimum orbital period of cataclysmic variables-Reference-Cited by-同舟云学术

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Evolution of rotationally and tidally distorted low-mass, close binary systems - Implications for the minimum orbital period of cataclysmic variables

Published:1985-12 Issue: Volume:299 Page:658
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Nelson L. A.,Chau W. Y.,Rosenblum A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 25 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Minimum Orbital Period of Precataclysmic Variables;The Astrophysical Journal;2018-10-16

2. WD 1202-024: the shortest-period pre-cataclysmic variable;Monthly Notices of the Royal Astronomical Society;2017-06-26

3. EPIC 220204960: A Quadruple Star System Containing Two Strongly Interacting Eclipsing Binaries;Monthly Notices of the Royal Astronomical Society;2017-01-19

4. EVOLUTION OF CATACLYSMIC VARIABLES AND RELATED BINARIES CONTAINING A WHITE DWARF;The Astrophysical Journal;2016-12-08

5. POPULATION SYNTHESIS OF CATACLYSMIC VARIABLES. I. INCLUSION OF DETAILED NUCLEAR EVOLUTION;The Astrophysical Journal;2015-08-12

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